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Radiation and Magnetic Pressure Support in Accretion Disks Around Supermassive Black Holes and the Physical Origin of the Extreme-Ultraviolet to Soft X-Ray Spectrum

Yan-Fei Jiang et al 2025 ApJ 988 43 Simulated black-hole disks with accretion rates between 0.03 and 4 times the Eddington rate are capable of reproducing the spectra seen from real disks, yielding…

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Kerry Hensley7mo agoen

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